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Title: Planck 2013 results. I. Overview of products and scientific results

Journal Article · · Astronomy and Astrophysics
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The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This report gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code given to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter ΛCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25σ. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations (σ8) derived from CMB data and that derived from Sunyaev-Zeldovich data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak. Analysis of Planck polarization data is not yet mature, therefore polarization results are not released, while the robust detection of E-mode polarization around CMB hot and cold spots is shown graphically.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Contributing Organization:
Planck Collaboration
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1523966
Journal Information:
Astronomy and Astrophysics, Vol. 571; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 1162 works
Citation information provided by
Web of Science

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Constraining the anisotropy of the Universe with the Pantheon supernovae sample journal November 2019
Probabilistic Forecasting of the Masses and Radii of Other Worlds journal December 2016
Modelling of the spectral energy distribution of Fornax A: leptonic and hadronic production of high-energy emission from the radio lobes journal December 2014
Bounds on higher derivative f(R,□R,T) models from energy conditions journal April 2019
The nature of submillimetre and highly star-forming galaxies in the EAGLE simulation journal June 2019
The multiphase circumgalactic medium traced by low metal ions in EAGLE zoom simulations journal August 2018
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples journal August 2014
Colloquium : Time-reversal violation with quantum-entangled B mesons journal February 2015
Size matters: abundance matching, galaxy sizes, and the Tully–Fisher relation in EAGLE journal October 2016
The Herschel Virgo Cluster Survey : XVIII. Star-forming dwarf galaxies in a cluster environment⋆ journal February 2015
Calibrated, cosmological hydrodynamical simulations with variable IMFs III: spatially resolved properties and evolution journal November 2018
Planck 2013 results. XXV. Searches for cosmic strings and other topological defects journal October 2014
The Herschel Virgo Cluster Survey: XX. Dust and gas in the foreground Galactic cirrus⋆⋆⋆ journal January 2017
Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations text January 2019
The New Numerical Galaxy Catalogue ( ν 2 GC ): properties of active galactic nuclei and their host galaxies journal November 2018
H.E.S.S. and Suzaku observations of the Vela X pulsar wind nebula journal July 2019
Detecting the neutral IGM in filaments with the SKA journal October 2019
Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update text January 2017
Bayesian inflationary reconstructions from Planck 2018 data journal November 2019
The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 journal March 2015
Baryogenesis and dark matter in U (1) extensions journal April 2017
The E-MOSAICS project: simulating the formation and co-evolution of galaxies and their star cluster populations journal December 2017
Theoretical Re-evaluations of Scaling Relations between SMBHs and Their Host Galaxies—1. Effect of Seed BH Mass journal September 2017
Decoherence, discord, and the quantum master equation for cosmological perturbations journal May 2017
Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. II. Second year of LP15 observations text January 2019
SU(2) cmb and the cosmological model: angular power spectra journal November 2018
Accuracy Of Estimating Highly Eccentric Binary Black Hole Parameters With Gravitational-Wave Detections text January 2018
Accuracy Of Estimating Highly Eccentric Binary Black Hole Parameters With Gravitational-Wave Detections text January 2018
Calibrating the cosmic distance scale ladder: the role of the sound-horizon scale and the local expansion rate as distance anchors journal March 2015
The evolution of the star formation rate function in the EAGLE simulations: a comparison with UV, IR and Hα observations from z ∼ 8 to z ∼ 0 journal August 2017
Testing the Cubic Galileon Gravity Model by the Milky Way Rotation Curve and SPARC Data journal April 2018
Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with ΛCDM journal May 2016

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